SDO HMI 2014-10-02 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.37 | 0.00 | 9.05 | -5.00 | 139.04 | -23.71 | 115.61 | 0.4463 | -793.4 | -692.9 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.43 | -4.40 | 140.79 | -21.97 | 116.15 | 0.4173 | -736.0 | -625.9 | |
| 0.00 | 1.76 | 0.00 | 0.96 | -4.59 | 139.93 | -22.82 | 115.66 | 0.4307 | -977.0 | -841.5 | |
| 0.00 | 2.11 | 0.00 | 1.17 | -5.81 | 139.39 | -23.36 | 117.59 | 0.4470 | -1034.0 | -833.6 | |
| 0.00 | 1.85 | 0.00 | 1.02 | -5.51 | 139.24 | -23.51 | 116.84 | 0.4469 | -927.0 | -827.2 | |
| 0.00 | 1.06 | 0.00 | 0.59 | -5.97 | 139.12 | -23.63 | 117.64 | 0.4519 | -651.0 | -621.4 | |
| 0.00 | 1.94 | 0.00 | 1.08 | -6.37 | 139.07 | -23.68 | 118.37 | 0.4556 | -855.0 | -769.9 | |
| 0.00 | 2.46 | 0.00 | 1.35 | -3.40 | 139.18 | -23.57 | 112.43 | 0.4336 | -812.0 | -636.8 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -3.61 | 139.18 | -23.57 | 112.88 | 0.4350 | -582.0 | -495.3 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -3.47 | 138.99 | -23.77 | 112.40 | 0.4369 | -867.0 | -656.3 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -6.57 | 138.23 | -24.52 | 117.89 | 0.4684 | -645.0 | -505.9 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -5.02 | 135.52 | -27.23 | 112.56 | 0.4955 | -641.0 | -485.5 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |